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High sensitivity SiO maser survey for mira variables

  • Section 2b: Solar-Stellar Connections
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Abstract

Simultaneous observations of the six transitions of SiO for 106 late-type stars were made. The SiO maser emission was detected in 83 stars. Thev=3 maser emission was detected in eight stars, and the29SiOv=0 emission in six stars. The29SiOv=0 emission is stronger and narrower than that of28SiO, suggesting that the29SiO emission is masing.

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References

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Authors and Affiliations

  1. Nobeyama Radio Observatory, Minamimaki, Nagano, Japan

    Se-Hyung Cho, Norio Kaifu, Nobuharu Ukita, Masaki Morimoto & Masahiko Hayashi

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  1. Se-Hyung Cho
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  2. Norio Kaifu
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  3. Nobuharu Ukita
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  4. Masaki Morimoto
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  5. Masahiko Hayashi
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Cho, SH., Kaifu, N., Ukita, N. et al. High sensitivity SiO maser survey for mira variables. Astrophys Space Sci 118, 237–239 (1986). https://doi.org/10.1007/BF00651131

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  • DOI: https://doi.org/10.1007/BF00651131

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